| 1 | spectral energy distribution | SED | 1441 | 100 | 2.001854 | 1504.03228,1504.00673,etc |
| 2 | cosmic microwave background | CMB | 958 | 90 | 1.00225 | 1504.01195,1504.05735,etc |
| 3 | active galactic nucleus | AGN | 2577 | 90 | 1.006123 | 1504.00362,1504.05583,etc |
| 4 | interstellar medium | ISM | 506 | 74 | 2.001502 | 1504.05735,1504.03261,etc |
| 5 | star formation rate | SFR | 1385 | 66 | 2.002769 | 1504.05583,1504.04454,etc |
| 6 | point spread function | PSF | 677 | 64 | 2.001464 | 1504.04024,1504.01832,etc |
| 7 | initial mass function | IMF | 451 | 63 | 2.000964 | 1504.04300,1504.04043,etc |
| 8 | sloan digital sky survey | SDSS | 758 | 61 | 2.002498 | 1504.02777,1504.04583,etc |
| 9 | signal to noise ratio | S/N | 456 | 48 | 1.001656 | 1504.02725,1504.05201,etc |
| 10 | dark matter | DM | 1756 | 41 | 2.008225 | 1504.01195,1504.04604,etc |
| 11 | nasa/ipac extragalactic database | NED | 84 | 40 | 1.000224 | 1504.04024,1504.05089,etc |
| 12 | markov chain monte carlo | MCMC | 194 | 39 | 1.000686 | 1504.03228,1504.04507,etc |
| 13 | gamma ray burst | GRB | 2107 | 39 | 2.009394 | 1504.00673,1504.02153,etc |
| 14 | field of view | FOV | 237 | 38 | 2.000808 | 1504.06530,1504.05089,etc |
| 15 | supernova | SN | 2704 | 37 | 2.011826 | 1504.06668,1504.04043,etc |
| 16 | very large array | VLA | 242 | 34 | 2.001198 | 1504.00673,1504.06282,etc |
| 17 | near infrared | NIR | 337 | 33 | 1.001259 | 1504.00446,1504.05592,etc |
| 18 | hubble space telescope | HST | 226 | 33 | 1.000821 | 1504.00228,1504.03299,etc |
| 19 | equivalent width | EW | 261 | 32 | 1.001269 | 1504.04043,1504.02725,etc |
| 20 | equation of state | EoS | 675 | 32 | 2.003639 | 1504.02506,1504.07631,etc |
| 21 | full width at half maximum | FWHM | 235 | 32 | 2.001214 | 1504.04507,1504.08001,etc |
| 22 | ultraviolet | UV | 880 | 32 | 2.004817 | 1504.00446,1504.07686,etc |
| 23 | black hole | BH | 1276 | 28 | 2.007991 | 1504.04300,1504.07592,etc |
| 24 | signal to noise | S/N | 179 | 27 | 1.00052 | 1504.00446,1504.05589,etc |
| 25 | star formation history | SFH | 459 | 27 | 1.002268 | 1504.06621,1504.00584,etc |
| 26 | large magellanic cloud | LMC | 381 | 27 | 1.00443 | 1504.06621,1504.00584,etc |
| 27 | cold dark matter | CDM | 421 | 26 | 2.002755 | 1504.02645,1504.02126,etc |
| 28 | kolmogorov smirnov | KS | 92 | 25 | 1.000346 | 1504.00363,1504.06282,etc |
| 29 | standard model | SM | 552 | 24 | 2.003688 | 1504.04024,1504.04604,etc |
| 30 | infrared | IR | 702 | 24 | 2.003093 | 1504.00248,1504.06887,etc |
| 31 | line of sight | LOS | 201 | 22 | 1.003988 | 1504.05735,1504.02135,etc |
| 32 | supermassive black hole | SBH | 258 | 22 | 1.003953 | 1504.05089,1504.02111,etc |
| 33 | white dwarf | WD | 427 | 21 | 2.00529 | 1504.01878,1504.04043,etc |
| 34 | three dimensional | 3D | 376 | 21 | 1.004009 | 1504.07631,1504.07659,etc |
| 35 | young stellar object | YSO | 240 | 21 | 1.002512 | 1504.05000,1504.06162,etc |
| 36 | local thermodynamic equilibrium | LTE | 309 | 21 | 1.001785 | 1504.07659,1504.06887,etc |
| 37 | intergalactic medium | IGM | 201 | 21 | 1.001916 | 1504.07686,1504.04620,etc |
| 38 | coronal mass ejection | CME | 770 | 21 | 2.009228 | 1504.04323,1504.06062,etc |
| 39 | general relativity | GR | 268 | 20 | 1.001805 | 1504.06805,1504.02455,etc |
| 40 | red giant branch | RGB | 196 | 20 | 2.001528 | 1504.01878,1504.03497,etc |
| 41 | large area telescope | LAT | 190 | 18 | 2.003164 | 1504.03228,1504.06343,etc |
| 42 | color magnitude diagram | CMD | 419 | 18 | 2.004747 | 1504.06621,1504.01742,etc |
| 43 | dark energy survey | DES | 439 | 18 | 1.004995 | 1504.03060,1504.02983,etc |
| 44 | asymptotic giant branch | AGB | 525 | 17 | 1.004793 | 1504.01878,1504.06098,etc |
| 45 | magnetohydrodynamic | MHD | 279 | 17 | 2.00353 | 1504.04323,1504.06120,etc |
| 46 | big bang nucleosynthesis | BBN | 86 | 16 | 1.001415 | 1504.04024,1504.04019,etc |
| 47 | navarro frenk white | NFW | 309 | 16 | 1.004159 | 1504.04019,1504.02510,etc |
| 48 | broad line region | BLR | 150 | 16 | 2.001172 | 1504.05638,1504.06190,etc |
| 49 | main sequence | MS | 313 | 16 | 2.002169 | 1504.01742,1504.00584,etc |
| 50 | probability distribution function | PDF | 107 | 16 | 1.000851 | 1504.00248,1504.03060,etc |
| 51 | very long baseline interferometry | VLBI | 210 | 16 | 1.003559 | 1504.00780,1504.01507,etc |
| 52 | square kilometre array | SKA | 163 | 16 | 2.004239 | 1504.08000,1504.00200,etc |
| 53 | two micron all sky survey | 2MASS | 205 | 16 | 2.001949 | 1504.06098,1504.03241,etc |
| 54 | cosmic ray | CR | 403 | 15 | 2.007856 | 1504.05735,1504.03261,etc |
| 55 | large synoptic survey telescope | LSST | 74 | 15 | 1.002012 | 1504.00673,1504.06088,etc |
| 56 | neutron star | NS | 361 | 15 | 2.002637 | 1504.02506,1504.03590,etc |
| 57 | far infrared | FIR | 231 | 15 | 1.003131 | 1504.05000,1504.06530,etc |
| 58 | radial velocity | RV | 322 | 15 | 2.002319 | 1504.05098,1504.03752,etc |
| 59 | milky way | MW | 407 | 15 | 1.003889 | 1504.01742,1504.06162,etc |
| 60 | polycyclic aromatic hydrocarbon | PAH | 199 | 15 | 1.003894 | 1504.05391,1504.03745,etc |
| 61 | japan society for the promotion of science | JSPS | 21 | 15 | 1.00011 | 1504.01594,1504.05589,etc |
| 62 | low mass x ray binary | LMXB | 72 | 15 | 2.000508 | 1504.06225,1504.05889,etc |
| 63 | horizontal branch | HB | 263 | 14 | 1.007914 | 1504.01878,1504.01742,etc |
| 64 | zero age main sequence | ZAMS | 67 | 14 | 1.000406 | 1504.01202,1504.07605,etc |
| 65 | small magellanic cloud | SMC | 435 | 14 | 1.004909 | 1504.06621,1504.07695,etc |
| 66 | colour magnitude diagram | CMD | 224 | 13 | 2.003226 | 1504.03520,1504.00584,etc |
| 67 | globular cluster | GC | 1245 | 13 | 2.006258 | 1504.01878,1504.01742,etc |
| 68 | deutsche forschungsgemeinschaft | DFG | 16 | 13 | 1.000159 | 1504.05000,1504.06162,etc |
| 69 | brightest cluster galaxy | BCG | 371 | 13 | 1.005228 | 1504.05583,1504.04583,etc |
| 70 | max planck institute for astronomy | MPIA | 13 | 13 | 1.000033 | 1504.02777,1504.03401,etc |
| 71 | very large telescope | VLT | 61 | 13 | 1.00064 | 1504.05391,1504.02469,etc |
| 72 | wide field camera 3 | WFC3 | 88 | 13 | 1.000731 | 1504.03299,1504.02101,etc |
| 73 | smoothed particle hydrodynamics | SPH | 120 | 13 | 2.001127 | 1504.00393,1504.03339,etc |
| 74 | canada france hawaii telescope | CFHT | 80 | 13 | 2.000993 | 1504.01734,1504.03320,etc |
| 75 | supernova remnant | SNR | 224 | 13 | 2.00297 | 1504.02246,1504.07238,etc |
| 76 | gravitational wave | GW | 336 | 12 | 2.003505 | 1504.04300,1504.02506,etc |
| 77 | adaptive optics | AO | 101 | 12 | 2.00331 | 1504.04043,1504.02933,etc |
| 78 | science and technology facilities council | STFC | 19 | 12 | 1.000213 | 1504.05583,1504.05206,etc |
| 79 | adaptive mesh refinement | AMR | 101 | 12 | 1.001129 | 1504.07754,1504.07458,etc |
| 80 | wide field infrared survey explorer | WISE | 217 | 12 | 2.003426 | 1504.00780,1504.04264,etc |
| 81 | baryon oscillation spectroscopic survey | BOSS | 56 | 12 | 1.00065 | 1504.02591,1504.03056,etc |
| 82 | weakly interacting massive particle | WIMP | 34 | 11 | 1.000441 | 1504.01195,1504.04019,etc |
| 83 | pre main sequence | PMS | 63 | 11 | 1.00069 | 1504.02766,1504.03299,etc |
| 84 | max planck institute for astrophysics | MPA | 14 | 11 | 1.00007 | 1504.02777,1504.03418,etc |
| 85 | luminosity function | LF | 145 | 11 | 2.001652 | 1504.06530,1504.06621,etc |
| 86 | ministry of economy and competitiveness | MINECO | 18 | 11 | 1.000315 | 1504.04583,1504.08001,etc |
| 87 | solar dynamics observatory | SDO | 57 | 11 | 2.00048 | 1504.04323,1504.06887,etc |
| 88 | dwarf spheroidal | dSph | 290 | 11 | 2.004349 | 1504.06621,1504.06673,etc |
| 89 | giant molecular cloud | GMC | 97 | 11 | 2.000891 | 1504.00647,1504.02095,etc |
| 90 | william herschel telescope | WHT | 56 | 11 | 2.000513 | 1504.06282,1504.08001,etc |
| 91 | full width half maximum | FWHM | 38 | 11 | 2.000327 | 1504.06282,1504.02962,etc |
| 92 | simple stellar population | SSP | 96 | 11 | 1.001214 | 1504.03299,1504.02983,etc |
| 93 | mid infrared | MIR | 291 | 11 | 2.003047 | 1504.01534,1504.03418,etc |
| 94 | synchrotron self compton | SSC | 127 | 10 | 1.001795 | 1504.03228,1504.04833,etc |
| 95 | two dimensional | 2D | 142 | 10 | 2.00175 | 1504.07659,1504.07534,etc |
| 96 | inverse compton | IC | 109 | 10 | 2.001152 | 1504.07592,1504.02014,etc |
| 97 | intracluster medium | ICM | 200 | 10 | 2.004291 | 1504.07754,1504.02095,etc |
| 98 | cerro tololo inter american observatory | CTIO | 86 | 10 | 2.001286 | 1504.00584,1504.06509,etc |
| 99 | position angle | PA | 161 | 10 | 1.003324 | 1504.06282,1504.02014,etc |
| 100 | one dimensional | 1D | 262 | 10 | 1.003275 | 1504.07534,1504.04857,etc |
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